---
abstract: 'Recent efforts on modeling coronal turbulence transport and shock acceleration
  self-consistently are reviewed. The considered models are based on the assumption
  that the turbulence responsible for the scattering of energetic ions consists of
  slab-mode Alfv\''en waves. A short discussion of the applied wave transport equation
  and particle transport coefficients is followed by a more extensive review of analytical
  and numerical modeling results of coupled evolution of energetic particle fluxes
  and wave intensities.'
adsnote: Provided by the SAO/NASA Astrophysics Data System
adsurl: https://ui.adsabs.harvard.edu/abs/2007AIPC..932..350V
authors:
- R. Vainio
- T. Laitinen
booktitle: Turbulence and Nonlinear Processes in Astrophysical Plasmas
category: publications
date: '2007-08-01'
doi: 10.1063/1.2778985
draft: false
editor:
- first: Dastgeer
  last: 'Shaikh'
- first: Gary
  last: 'Zank'
  middle: P.
featured: false
month: August
pages: 350-355
projects: []
publication: Turbulence and Nonlinear Processes in Astrophysical Plasmas
publication_types:
- '2'
series: American Institute of Physics Conference Series
tags:
- Mhd waves
- Plasma waves turbulence
- Energetic particles
- Coronal mass ejection
title: 'Turbulence transport and shock acceleration in solar corona'
type: INPROCEEDINGS
volume: '932'
year: '2007'
---